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Role of tides on the formation of the Antarctic Slope Front at the Weddell-Scotia Confluence

机译:潮汐对Weddell-Scotia汇合处南极斜坡前锋形成的作用

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摘要

© 2015. American Geophysical Union. All Rights Reserved. California Institute of Technology. Government sponsorship acknowledged. The structure of the Antarctic Slope Front (ASF) and the associated Antarctic Slope Current (ASC) on the Scotia Sea side of the Weddell-Scotia Confluence (WSC) is described using data from a hydrographic survey and three 1 year long moorings across the continental slope. The ASC in this region flows westward along isobaths with an annual mean speed of ∼0.2 m s, with time variability dominated by the K and O tidal diurnal constituents, a narrowband oscillation with ∼2-week period attributable to the spring/neap tidal cycle, and seasonal variability. Realistic and idealized high-resolution numerical simulations are used to determine the contribution of tides to the structure of the ASF and the speed of the ASC. Two simulations forced by realistic atmospheric forcing and boundary conditions integrated with and without tidal forcing show that tidal forcing is essential to reproduce the measured ASF/ASC cross-slope structure, the time variability at our moorings, and the reduced stratification within the WSC. Two idealized simulations run with tide-only forcing, one with a homogeneous ocean and the other with initial vertical stratification that is laterally homogeneous, show that tides can generate the ASC and ASF through volume flux convergence along the slope initiated by effects including the Lagrangian component of tidal rectification and mixing at the seabed and in the stratified ocean interior. Climate models that exclude the effects of tides will not correctly represent the ASF and ASC or their influence on the injection of intermediate and dense waters from the WSC to the deep ocean. Key Points: Tides set mean properties of Antarctic Slope Front in Weddell-Scotia Confluence Volume convergence by tidal rectification, plus mixing, creates Slope Current Shelf water properties in Weddell-Scotia Confluence modified by tides
机译:©2015。美国地球物理联盟。版权所有。加州理工学院。政府赞助得到承认。韦德—斯科舍汇流处(WSC)斯科舍海侧的南极斜坡前缘(ASF)以及相关的南极斜坡潮流(ASC)的结构是使用水文勘测数据和整个大陆上的三个为期一年的系泊设备描述的坡。该区域的ASC沿等压线向西流动,年平均速度约为0.2 ms,时间变化主要受潮汐日和昼夜分量的影响,春季/潮汐周期约为2周,为窄带振荡,和季节性变化。现实和理想的高分辨率数值模拟用于确定潮汐对ASF结构和ASC速度的贡献。由现实的大气强迫和边界条件(有或没有潮汐强迫)强迫进行的两个模拟表明,潮汐强迫对于重现测得的ASF / ASC横坡结构,系泊设备的时间变化以及减少WSC内部分层至关重要。两种仅在潮汐作用下进行的理想化模拟,一个具有均质的海洋,另一个具有横向均质的初始垂直分层,表明潮汐能通过沿包括拉格朗日分量在内的效应所引发的斜坡上的体积通量收敛而产生ASC和ASF。海底和分层海洋内部的潮汐整流和混合过程。排除潮汐影响的气候模型将不能正确地代表ASF和ASC或它们对从WSC向深海注入中,浓水的影响。要点:潮汐设定了韦德尔-斯科舍河合流处南极坡锋的平均性质,通过潮汐整流和混合,使体积收敛,形成了经潮汐修正的韦德尔-斯科舍省合流处的斜坡流架子水性质。

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